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Authordc.contributor.authorGálvez Ortiz, M. C.
Authordc.contributor.authorKuznetsov, M.es_CL
Authordc.contributor.authorClarke, J. R. A.es_CL
Authordc.contributor.authorPavlenko, Ya. V.es_CL
Authordc.contributor.authorFolkes, S. L.es_CL
Authordc.contributor.authorPinfield, D. J.es_CL
Authordc.contributor.authorJones, H. R. A.es_CL
Authordc.contributor.authorJenkins, James Stewartes_CL
Authordc.contributor.authorBarnes, J. R.es_CL
Authordc.contributor.authorBurningham, B.es_CL
Authordc.contributor.authorDay Jones, A. C.es_CL
Authordc.contributor.authorMartín, E. L.es_CL
Authordc.contributor.authorGarcía Pérez, A. E.es_CL
Authordc.contributor.authorBurgo, C. deles_CL
Authordc.contributor.authorPokorny, R. S.es_CL
Admission datedc.date.accessioned2014-12-29T15:21:54Z
Available datedc.date.available2014-12-29T15:21:54Z
Publication datedc.date.issued2014
Cita de ítemdc.identifier.citationMNRAS 439, 3890–3907 (2014)en_US
Identifierdc.identifier.otherdoi:10.1093/mnras/stu241
Identifierdc.identifier.urihttps://repositorio.uchile.cl/handle/2250/126820
General notedc.descriptionArtículo de publicación ISIen_US
Abstractdc.description.abstractWe present a study of age-related spectral signatures observed in 25 young low-mass objects that we have previously determined as possible kinematic members of five young moving groups: the Local Association (Pleiades moving group, age = 20.150 Myr), the Ursa Major group (Sirius supercluster, age = 300 Myr), the Hyades supercluster (age = 600 Myr), IC 2391 supercluster (age = 35.55 Myr) and the Castor moving group (age = 200 Myr). In this paper we characterize the spectral properties of observed high- or low-resolution spectra of our kinematic members by fitting theoretical spectral distributions. We study signatures of youth, such as lithium I 6708A, H[alfa] emission and other age-sensitive spectroscopic signatures in order to confirm the kinematic memberships through age constraints. We find that 21 (84 per cent) targets show spectroscopic signatures of youth in agreement with the age ranges of the moving group to which membership is implied. For two further objects, age-related constraints remain difficult to determine from our analysis. In addition, we confirm two moving group kinematic candidates as brown dwarfs.en_US
Patrocinadordc.description.sponsorshipMCGO acknowledges financial support by the Spanish MICINN under the Consolider-Ingenio 2010 Program grant CSD2006- 00070: First Science with the GTC (http://www.iac.es/consolideringenio- gtc). She also acknowledges the support of a JAE-Doc CSIC fellowship co-funded with the European Social Fund under the program ‘Junta para la Ampliaci´on de Estudios’. The work of MKK and YaVP was supported by EU PF7 Marie Curie Initial Training Networks (ITN) ROPACS project (GA N 213646). Financial support was also provided by the Spanish Ministerio de Ciencia e Innovaci´on and Ministerio de Econom´ıa y Competitividad under AyA2011- 30147-C03-03 grant. SLF acknowledges funding support from the ESO-Government of Chile Mixed Committee 2009, and from the GEMINI–CONICYT grant 32090014/2009. JSJ acknowledges funding by Fondecyt through grant 3110004 and partial support from CATA (PB06, Conicyt), the GEMINI-CONICYT FUND and from the Comit´e Mixto ESO-GOBIERNO DE CHILE. Financial support was also provided by theMexican research council (CONACYT) grant.en_US
Lenguagedc.language.isoenen_US
Publisherdc.publisherOxford University Pressen_US
Type of licensedc.rightsAttribution-NonCommercial-NoDerivs 3.0 Chile*
Link to Licensedc.rights.urihttp://creativecommons.org/licenses/by-nc-nd/3.0/cl/*
Keywordsdc.subjectbrown dwarfsen_US
Títulodc.titleSpectroscopic signatures of youth in low-mass kinematic candidates of young moving groupsen_US
Document typedc.typeArtículo de revista


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Except where otherwise noted, this item's license is described as Attribution-NonCommercial-NoDerivs 3.0 Chile